Fig. C.1.
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Evolution of the envelope mass of the primary star in the models with qi = 0.95 as a function of time prior to core collapse (left) and the different contributors to its removal (right): growth of the helium core (top), mass-loss by winds (middle) and mass-loss by mass-transfer (bottom). The colors, dashing, and shading are the same as in Fig. 2.
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